Many common Skyrme functionals present ferromagnetic instabilities or unrealistic density dependence of the spin-dependent Landau parameters. To solve these problems, we consider the Skyrme interaction as a density-functional rather than a density-dependent two-body force. This allows us to adjust the spin-dependent terms of the extended Skyrme functionals of our previous paper [M. Duan and M. Urban, Phys. Rev. C 110, 065806 (2024)] independently without altering the properties of spin-saturated matter. The parameters of the spin-dependent terms are determined by fitting the Landau parameters $G_0$ and $G_0^{\prime }$ in neutron matter and symmetric nuclear matter and the effective-mass splitting of up and down particles in spin-polarized matter to the results of microscopic calculations. Using these parametrizations, called Sky3s and Sky4s, the spin-related properties of nuclear matter are in good agreement with the microscopic results. As an application, we compute response functions and neutrino scattering rates of neutron-star matter with these functionals having realistic effective masses and Landau parameters.

Close

PrevNext

View figure in article

• Nuclear matter in neutron stars
• Nuclear density functional theory